Comparative study of the \(2:3\) and \(3:4\) resonant motion with Neptune: an application of symplectic mappings and low frequency analysis
From MaRDI portal
Publication:1766785
DOI10.1023/B:CELE.0000023391.85690.31zbMath1160.70331OpenAlexW2043905874MaRDI QIDQ1766785
Thomas Kotoulas, George Voyatzis
Publication date: 1 March 2005
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1023/b:cele.0000023391.85690.31
Related Items
On families of periodic solutions of the restricted three-body problem, Long-term orbital dynamics of trans-Neptunian objects, Retrograde periodic orbits in 1/2, 2/3 and 3/4 mean motion resonances with Neptune, Neptune's resonances in the scattered disk, Periodic solutions of the restricted three-body problem for a small mass ratio, Geometrical properties of local dynamics in Hamiltonian systems: the generalized alignment index (GALI) method, The phase space structure of retrograde mean motion resonances with Neptune: the 4/5, 7/9, 5/8 and 8/13 cases, A non-planar circular model for the 4/7 resonance
